Measurement of sin2θW using e+e pairs from pp collisions at √s = 1.96 TeV
28 Jun 2016

Phys Rev D93, 112016 (2016)
arXiv:1605.02719[hep-ex]

W. Sakumoto, A. Bodek, and J.-Y. Han
University of Rochester



Abstract

Drell-Yan lepton pairs are produced in the process pp → γ*/Z + X, with the subsequent decay of the γ*/Z into lepton pairs. The angular distribution of decay electrons provides information on the electroweak-mixing parameter sin2θW via its observable effective-leptonic sin2θW or sin2θefflept. The measurement uses 9.4 fb-1 of CDF Run II data in the e+e channel where the pairs are in the mass range above 50 GeV. The value of sin2θefflept is found to be 0.23248 ± 0.00053. When combined with the previous CDF measurement using μ+μ pairs, the result is 0.23221 ± 0.00046.

Introduction

The Drell-Yan process at tree level consists of two parton level diagrams: qq → γ* and Z → e+e. Fermions (f) couple to the virtual photon via vector coupling, Qfγμ, where Qf is the fermion charge (in units of e). The fermion coupling to a Z boson has both vector (V) and axial (A) couplings: gVfγμ + gAfγμγ5. The Born couplings are:

where T3f is the third component of the fermion weak isospin. These couplings affect the lepton angular distributions.

The angular distribution of the leptons is analyzed in the Collins-Soper (CS) rest frame of the ee-pair. The polar angle of the e is denoted as θ, and the azimuthal angle as φ. In the CS frame, the placement of the z axis is approximately along the direction of the incoming quark. When the ee-pair transverse momentum, PT is zero, the CS and lab coordinates are the same. The angular distribution integrated over φ is

where A0 and A4 are called angular distribution coefficients, and they are ratios of γ*/Z helicity cross sections relative to the unpolarized cross section. A0 appears at NLO with QCD radiation, so it is zero at PT=0.

The A4 coefficient is parity violating, non-zero at PT=0, and induces an asymmetry in the cosθ distribution. It is a consequence of vector and axial current interference, and there are two sources: γ*-Z interference and the Z boson vector and axial-vector interference. The γ*-Z interference depends on gA (T3). The Z boson vector and axial-vector interference includes gV, so at tree level, the A4 contribution from it is proportional to gVlgVq

where Ql is the lepton charge and Qq is the quark charge. Loop and vertex electroweak radiative corrections modify the Born-level T3f and sin2θW couplings by a few percent, and so effective couplings are observed. As sin2θW ∼ 0.223, A4 is most sensitive to the effective lepton-Z coupling which is denoted as sin2θefflept. A 1% variation of sin2θW results in a 8% change in the lepton-Z factor (containing Ql), and a change of 1.5% in the quark-Z factor (containing Qq) for u-quarks, and of 0.4% for d-quarks.


In this analysis, the forward-backward cosθ asymmetry of the electron pairs is measured as a function of their mass. The asymmetry is defined as:

where σ+ is the total cross section for cosθ≥0, and σ the corresponding cross section for cosθ<0.

This plot on the left illustrates the typical behavior of Afb as a function of the lepton-pair mass M. The vertical line is at M=MZ. The label u+d denotes the overall asymmetry. The labels u and d denote the contributions to the overall asymmetry from charge +2/3 and −1/3 quarks, respectively. The denominator for all cases is the total cross section from quarks of all charges. The intercepts at M=MZ are related to sin2θW. The rise and fall away from M=MZ is from γ*-Z interference and is influenced by the PDFs. These dependencies are illustrated here.
The method used to derive sin2θefflept has two components: the measurement of Afb and calculations of Afb for various input values of sin2θW. The measured Afb is compared to the calculated Afb templates to determine the value of sin2θefflept that best describes the measurement. The calculation of Afb are QCD calculations that use LEP-like implementations of electroweak radiative corrections. These corrections are form factors to the tree-level T3f and sin2θW couplings, and they are 1 to 4% in value [ PRD 88, 072002 ].

Electron Analysis

The Data

The electron candidates used in this analysis can be in either the CDF central (C) or the forward end plug (P) calorimeters. The central and plug calorimeters cover the range, |ηdet|<1.1 and 1.1<|ηdet|<3.5 respectively. Each electron is required to have an associated track and pass standard CDF electron selection and fiducial cuts. Three electron-pair topology categories are used with the following kinematic selections.

  1. Central-central (CC)
  2. Central-plug (CP)
  3. Plug-plug (PP)

PP topology ee-pairs are not used in the measurement of Afb because of the high charge misidentification rate of tracking in the forward region. However, PP topology ee-pairs are used for energy calibrations. For CP ee-pairs, the central leg is used to identify the e. For CC pairs, only opposite-charge pairs are used in the measurement of Afb. The same-charge pairs are primarily composed of a large QCD background and Z's with the charge of one electron misidentified.

The Simulation

PYTHIA 6.2 simulates the tree level process qq → γ*/Z → ee followed by parton showering. This is followed by CDF II event and detector simulations. The event simulation includes PHOTOS 2.0 which adds final state QED radiation (QED FSR) to charged particle vertices. The simulated events are selected, reconstructed, as analyzed as the data. The generator-level PT distribution of the γ*/Z boson is adjusted so that the simulated PT distribution is the same as in the data. This is done in two rapidity bins. In addition, the mass distribution at the generator level is adjusted with a calculated K-factor: ResBos (CTEQ6.6) to Pythia (CTEQ5L).

Corrections to the Data and Simulation

The same event selection criteria are applied to both the data and the simulated data. Corrections are applied to both the data and simulated data for the measurement of Afb. Event rate corrections are applied to the simulation to normalize its rates with respect to the data. In particular, the pp collision vertex distributions that affect energy calibrations are corrected. The distribution of the number of vertices per event and the location of the collision along the beamline are adjusted so that they agree with the observed distributions.

The energy scale of the data and simulation are calibrated with an adaptation of the technique used to calibrate the muon momentum in the previous measurement of Afb [PRD 89,072005 (2014), and A. Bodek, Eur. Phys. J. C 67, 321 (2010)]. With this technique, the Z-boson pole mass location in the ee-pair mass distributions of the data and simulation are aligned with the equivalent generator level quantity. The generator level electrons are after QED FSR, are clustered with nearby photons, and their corresponding reconstruction level electrons pass all selection requirements. As there are 1440 calorimeter towers with time-dependent gains, the calibration is done in a series of iterative steps. Time and position dependence of the gains of the data and simulation are removed with the calibrations. The calibrations for the simulation also include the tuning of the calorimeter resolutions so that they agree with those observed in the data.

Because of the track requirement on each electron, the backgrounds are very small in the Z-peak region and do not affect the energy calibrations. However, they are larger at low and high masses. The QCD background shape and level for each of the three ee-pair topologies are derived from the ee-pair mass distributions of the data. EWK backgrounds from WW, WZ, ttbar, W+jets, and Z → ττ are from Monte Carlo (MC) samples which are simulated and reconstructed as data. The difference between the data and the sum of the simulated signal and EWK backgrounds is taken as the QCD background. The QCD background is extracted from a fit over the mass region, 42-400 GeV. The QCD background sample used for background subtractions is derived from the data set used to select ee-pairs for the measurement. However, some of the selections are reversed to obtain a jet or hadron like sample of pairs. As the reverse selection biases the mass distribution, it is reweighted to match the background shape and level obtained in the fit to the data. The results of the background fits are shown below.

CC opposite-charge pair mass distribution. The data are the crosses and the red histogram the sum of the simulation and all backgrounds. The backgrounds are: QCD (magenta), Z → ττ (green), W+jets (blue), WW+WZ+ZZ (cyan), and tt (purple). The χ2 between the data and sum of the simulation and backgrounds is 56 for 50 bins.

CP pair mass distribution. The data are the crosses and the red histogram the sum of the simulation and all backgrounds. The backgrounds are: QCD (magenta), Z → ττ (green), W+jets (blue), WW+WZ+ZZ (cyan), and tt (purple). The χ2 between the data and sum of the simulation and backgrounds is 50 for 50 bins.

The CC, CP, and PP samples contain 227, 258, and 80 thousand events respectively. The corresponding fractions of background over the 42-400 GeV range are: 1.1%, 1.2%, and 2.1% for the CC, CP, and PP topologies. For the CC and CP samples, the backgrounds under the Z peak is small, and away from the peak, the level increases from 0.1% to 10%. The PP sample is only used in calibrations (which uses events in the Z-peak region). Backgrounds are subtracted on an event-by-event basis for the measurement of Afb, which is for M > 50 Gev (or ln M > 3.9).

The following show the results of the energy calibrations and background fits for the CC and CP topology ee-pairs.
CC opposite-charge pair mass distribution. The crosses are the background subtracted data, and the histogram the simulated Z's. The χ2 between the data and sum of the simulation and backgrounds is 214 for 200 bins.

CP pair mass distribution. The crosses are the background subtracted data, and the histogram the simulated Z's. The χ2 between the data and sum of the simulation and backgrounds is 235 for 200 bins.

CC same-charge pair mass distribution. The crosses are the background subtracted data, and the histogram is the simulated γ*/Z's with charge misidentification. Charge misidentification is reproduced well by the simulation, and so charge misidentification for the CP events is also expected to be properly accounted by the simulation.

ET distribution for the CC topology electron with the larger ET. The crosses are the background subtracted data, and the histogram the simulated Z's.

ET distribution for the CP topology electron with the larger ET. The crosses are the background subtracted data, and the histogram the simulated Z's.

The Afb Measurement

The traditional method to measure Afb utilizies corrected cross sections, σ = N/(LεA), where L is the integrated luminosity, ε the reconstruction efficiency, and A the acceptance. The fully corrected forward-backward asymmetry is given by

The forward-backward asymmetry is measured using the event weighting method [A. Bodek et al., Eur. Phys. J. C 72, 2194 (2012)], which is equivalent to measurements of Afb in bins of |cosθ| with the assumption that (εA)+ = (εA), or equivalently that the detector is charge symmetric. Thus, the asymmetry in a bin is [N+−N] /[N++N]. The numerator event difference is proportional to 2A4|cosθ|, the denominator event sum is proportional to 2(1+cos2θ + ..), and the ratio, or the measured asymmetry in the bin is A4ζ, where ζ = |cosθ|/(1+cos2θ + ..). The measurements of Afb in |cosθ| bins/regions is reformulated to an unbinned measurement with event weights: where the n and d subscripts denote different and separately weighted event sums. Consider the events in a fixed |cosθ| region. They must have a numerator weight to compensate the |cosθ| angular dependence of the numerator event difference, and a denominator weight to compensate the (1+cos2θ + ..) angular dependence of the denominator event sum. Both the numerator and denominator events weights must contain the factor ζ2 for the statistical combination of these events with those from other |cosθ| regions. The method is equivalent to using a maximum likelihood method, and is expected to improve the statistical precision of the measurement by about 20%. The event-weighting method does not compensate the following: These require separate and additional compensation.
Afb slowly increases as |y| increases beyond |y|=1. Consequently, as the angular weighting method requires events for account for this, the measurement must be restricted to a region where there is sufficent acceptance. Thus, the boson rapidity is restricted to |y| < 1.7. This also limits the size of secondary acceptance corrections. The curve labeled PYTHIA shows the (arbitrarily normalized) shape of the underlying rapidity distribution from PYTHIA.
The acceptance and non-uniformity corrections are small.
The raw Afb measurement is shown in the plot on the left, along with the PYTHIA prediction (before QED FSR). The underflow bin is 50-64 GeV/c2 and the overflow bin is 150-350 GeV/c2. Only event weighting acceptance corrections are applied.

The event weighted sums N±n and N±d require resolution unfolding in the electron-pair mass and cosθ. The simulation is used to do the unfolding. Bin-to-bin event migrations are tracked by the smearing transfer matrix ngr, which tabulates the number of selected events produced in mass bin g that are reconstructed in another mass bin r. The following estimator is used as the resolution unfolding matrix: ngr/Nr, where Nr is the total number of events reconstructed in mass bin r. Because of the different energy resolutions of CC and CP electron pairs, separate transfer matrices are maintained for each topology. The transer matrices also used to estimate the Afb measurement covariance matrix. The separate CC and CP unfolding is combined for the covariance matrix. This method of unfolding requires that the simulated data cosθ distribution match the data. The simulated data cosθ distribution is tuned to match the data. Only adjustments symmetric in cosθ are applied, and the intrinsic asymmetry is unchanged. The default φ distribution is adequately simulated.

The final step of the Afb measurement after the resolution unfolding, is the correction of the small biases after event-weighting and unfolding. They are primarily due to regions of limited kinematic acceptance and detector non-uniformities. The simulation is used to predict the bias, defined as the true value minus the estimate of Afb from the event-weighting method after resolution unfolding. The true value is the PYTHIA calculation of Afb with the boson rapidity kinematic restriction of |y| < 1.7. The estimate is the Afb obtained with the simulated data. All corrections applied to the data are applied to the simulated data.

The black crossses are the correction for uncompensated biases after event weighting and resolution unfolding. The significant bias corrections to Afb are under 8% in magnitude and most are 3% or less. The estimated Afb is the event-weighted simulated data after unsmearing.

The blue histogram in the bias plot above is the Pythia calculation of Afb(|y|<1.7)−Afb(|y|<1.5), and the uncertainties shown are from PDFs. It is representative of the bias from rapidity regions with limited acceptance; it is the bias correction for a detector with zero acceptance for |y|>1.5.

The fully corrected Afb measurement is obtained by adding the bias correction to the event weighted and unsmeared Afb.

Fully corrected Afb. The first bin, denoted as the 'underflow' bin, covers the mass range 50-64 GeV. The last bin, denoted as the 'overflow' bin covers the mass range 150-350 GeV. The uncertainties shown are bin-by-bin unfolding estimate, and not the diagonal elements of the measurement covariance matrix. The vertical line is the mass of the Z-boson. The PYTHIA prediction is with sin2θefflept = 0.232. The Powheg-Box prediction, described in the next section, uses sin2θW = 0.2243 (sin2θefflept = 0.2325).

QCD Calculations:

a) Electroweak radiative corrections

QCD, QED, and weak radiative corrections can be organized to be separately gauge invariant, and corrections for each can be applied separately and independently. QED radiative corrections (with real photons) are not included in the calculation of Afb. They are included in the simulation physics model, so QED radiative effects are removed from the measurement of Afb.

Weak radiative corrections are based on ZFITTER 6.43's e+e → Z → qq amplitude form factors. The ZFITTER form factors are finite and gauge invariant. Thus photon corrections that involve massive gauge bosons are included in the Z amplitude form factors for gauge invariance. Internal QED radiative corrections to the photon propagator are only from fermion loops, and this correction is another form factor. ZFITTER uses the on-shell renormalization scheme for its form factors. All particle masses are on shell, and sin2θW = 1 − MW2/MZ2 to all orders of perturbation theory. The values of the form factors depend on the input sin2θW and other standard model parameters.

b) Drell-Yan QCD calculations

The ZFITTER complex-valued form factors are incorporated into QCD calculations for an enhanced Born approximation (EBA) to the electroweak couplings. For the form factors, √s is assigned the mass of the lepton pair. This done for both LO and NLO QCD calculations of the Drell-Yan process. Operationally, the QCD related portion of matrix elements are unchanged, and only the electroweak coupling portions need to be appropriately modified. Two NLO calculations are used in the calculations of Afb: Powheg-Box and ResBos. The Powheg-Box calculation is interfaced with Pythia's parton showering algorithm, and for brevity, the Powheg-Box plus Pythia combination is denoted as Powheg-Box. A simple QCD LO, or tree calculation of the Drell-Yan process is used as a baseline reference for the higher order QCD calculations. For the Powheg-Box and LO calculations, the NNPDF-3.0 NNLO PDF ensemble is used (αs = 0.118). The ResBos calculation uses CTEQ6.6. The EBA form factors modifies the Born gA and gV couplings:

where ρ and κ are s-dependent, complex valued, and fermion charge and weak iso-spin dependent form factors. The combination, κ sin2θW is called an effective sin2θW, and the measured Afb is directly related to this combination, and in particular, most sensitive to the one at the lepton vertex. The κ form factor is different for the l-Z and q-Z vertex. Its reference value, for comparisons with LEP measurements, is the real part at √s = MZ. That is, its value at the Z pole.

The Powheg-Box NLO predictions of Afb for various input values of sin2θW are chosen as the default for comparisons with the measurement. The ResBos and LO calculations are for comparisons and cross checks.

The NNPDF-3.0 PDFs are an ensemble of a 100 probability-based PDFs. They are random samples from the probabilty density distribution of the PDF parameters constrained by measurements. Each PDF of the ensemble is equally probable. Thus, the prediction for an observable is the simple average of the values calculated over the ensemble, and the uncertainty of the observable from PDFs is the rms about the average. If a new measurement is consistent with those used to constrain the PDF parameters, it can be incorporated into the ensemble without regeneration. This is accomplished by re-weighting the ensemble PDFs, numbered 1 to N, with the probabilities of likelihood between the new measurement and the calculations:

where wk is the weight is for the kth PDF of the ensemble. Thus, the simple average and rms are replaced with a weighted average and rms. This is denoted as the Giele-Keller (GK) weighting method [ PRD 58, 094023 (1998) ]. For the Powheg-Box and Tree calculation ensemble averages with NNPDF-3.0 PDFs, the GK-weighted average and rms are selected for the results.

Extraction of sin2θefflept

The fully corrected Afb measurement is compared with predictions using the χ2 statistical measure derived from the measurement error matrix. The error matrix is regulated with a cutoff function. The SVD (singular value decompositon) expansion of the covariance or error matrix in terms of the eigenvalues and eigenvector projection operators of the covariance matrix has eigenvalues that are orders of magnitude smaller than the smallest uncertainty of the measurement. This produces instabilities in the χ2 and the cutoff function attenuates those instabilities.

For the EBA-based QCD calculations, the parameter that specifies the electroweak mixing is sin2θW. As the measurement is directly sensitive to sin2θefflept, the best-fit value of sin2θW only represents the corresponding sin2θefflept, which is independent of the standard model parameters used for the EBA form factors. However, the interpretation of the best-fit value of sin2θW only has meaning within the context of the model assumptions used.

The χ2 is calculated for a series of Afb calculations, denoted as scan templates. The series of scan points are fit to a generic χ2 functional form

where the terms with the overlines are fit parameters. The sin2θW parameter is the extracted (best-fit) value of sin2θW, and σ the corresponding measurement uncertainty. The χ2, relative to 15 mass bins, is the χ2 goodness-of-fit for the extracted value.

An example of the χ2 scan over the Powheg-Box NLO templates. The inverted triangles are the scan points, and the solid curve is the fit to those scan points.


The results of the template scans are summarized in the table below.

Template
(Measurement)
sin2θefflept sin2θW PDF χ2
Powheg-Box NLO, NNPDF-3.0 0.23248±0.00049 0.22428±0.00048 ±0.00018 15.4 (15)
ResBos NLO, CTEQ6.6 0.23249±0.00049 0.22429±0.00047
21.3 (15)
Tree LO, NNPDF-3.0 0.23250±0.00049 0.22430±0.00047 ±0.00021 21.5 (15)
Pythia, CTEQ5L 0.23207±0.00046
24.6 (15)
(CDF 9.2 fb−1 Afb(μμ)) 0.2315±0.00010 0.2233±0.00009
21.1 (16)
(CDF 2.1 fb−1 A4(ee)) 0.2328±0.0011 0.2246±0.0011
(LEP-1 and SLD AFB0,b) 0.23221±0.00029
(SLD Al) 0.23098±0.00026

The template scan uncertainties are statistical only. The PDF column is the uncertainty from NNPDF-3.0. In the χ2 column, the number in parenthesis is the number of mass bins. Also included are previous measurements: CDF ee A4 PRD 88, 072002, CDF μμ Afb PRD 89, 072005, and LEP-1+SLD [S. Schael et al. (ALEPH, DELPHI, L3, OPAL, and SLD Collaborations), Phys. Rep. 427, 257 (2006)]. The LEP-1 and SLD measurements listed are the most precise of their individual measurements; the Al based measurement is from purely leptonic states.

While the sin2θW values from Powheg-Box and ResBos calculations are the same, the χ2 values differ. The Afb difference relative to the Pythia CTEQ5L calculation (sin2θefflept = 0.232), ΔAfb = Afb − Afb (Pythia), shows differences in the best-fit Afb.
ΔAfb for the measurement, the Powheg-Box Afb with the default PDF of NNPDF-3.0, and the ResBos Afb with CTEQ6.6. The ΔAfb=0 line is Pythia with CTEQ5L. The uncertainties are the bin-by-bin unfolding estimates, which are correlated in the Z-pole region. However, this illustrates the dependence of the Afb measurement to PDFs.

The Powheg-Box template fit parameters of χ2 vs sin2θW for all of the ensemble PDFs of NNPDF-3.0. The Afb measurement and templates span 15 mass bins. This illustrates that the measurement is consistent with the other input measurements of NNPDF-3.0.

Uncertainities of the Extracted sin2θefflept

The uncertainties to sin2θefflept are from the measurement of Afb and the template predictions of Afb. For the measurement, these sources are considered: the electron energy scale plus resolution, and the backgrounds. For the predictions, two source are considered: QCD scales and NNPDF-3.0 PDFs. For the inference of sin2θW based on the measurement, the uncertainty of the top mass input to ZFITTER is considered.

The relative difference between simulation and data energy scales allowed by the data is taken as the energy scale uncertainty. The energy scale and resolution of central and plug electrons are well constrained by the precision of the Z-peak within the electron-pair mass distribution. The uncertainties of the energy scale and background fits are propagated to the extracted value of sin2θW. The effect from limitations of the energy resolution model in the simulation is estimated to be negligible.

The QCD scale undertainty is taken to be difference between the Powheg-Box NLO and Tree (LO) values of sin2θW.

The value of the inferred sin2θW based on the measurement depends on the SM input parameters of ZFITTER. The influence of the top mass measurement uncertainty, 173.2±0.9 GeV/c2, is included as a systematic uncertainty. This uncertainty is denoted as the form factor uncertainty.

The uncertainties are summarized in the table below. In this table, 'Data' denotes the uncertainties from the Afb measurement, and 'Pred' denotes the prediction uncertainties.

Source sin2θefflept sin2θW
Data: Measurement±0.00049 (stat) ±0.00048 (stat)
Data: Energy scale±0.00003 (syst) ±0.00003 (syst)
Data: Backgrounds±0.00002 (syst) ±0.00002 (syst)
Pred: QCD scales±0.00002 (syst) ±0.00002 (syst)
Pred: QCD PDFs±0.00019 (syst) ±0.00018 (syst)
Pred: Form factor ±0.00008 (syst)


Results

The results of the extraction are summarized below.

where the first uncertainty is the statistical uncertainty, and the second is the systematic uncertainty. All systematic uncertainties are included and combined in quadrature.

The interpretation of sin2θW and MW only has meaning within the context of the standard model parameters used for the EBA form factors. The context is similar to the environment for standard model fits of Z-pole measurements by LEP-1/SLD [Phys. Rep. 427, 257 (2006)], but with the exception that the Higgs boson mass parameter is set to 125 GeV/c2.


Combination of Electron and Muon Results

The Afb measurement using ee-pairs and the previous CDF measurement using μμ-pairs PRD 89, 072005 are over different kinematic ranges: |yee| < 1.7 and |yμμ| < 1. For the combined result on the electroweak-mixing parameter sin2θefflept (sin2θW), Afb templates are calculated separately, and the joint χ2 of the individual comparisons used to extract the combined electroweak-mixing parameters.

The results of the combination are summarized in the table below. The methods of evaluation for the χ2 between the Afb measurements and its templates are unchanged. The Powheg-Box NLO and Tree calculations utilize the NNPDF-3.0 ensemble of PDFs.

Template sin2θefflept sin2θW PDF χ2
Powheg-Box NLO 0.23221±0.00043 0.22400±0.00041 ±0.00016 35.9 (31)
Tree LO 0.23215±0.00043 0.22393±0.00041 ±0.00016 37.4 (31)

The template scan uncertainties are statistical only. The PDF column is the uncertainty from NNPDF-3.0. In the χ2 column, the number in parenthesis is the number of mass bins. The electron and muon channels have 15 and 16 mass bins, respectively.
The Powheg-Box fit parameters of χ2 vs sin2θW for all of the ensemble PDFs of NNPDF-3.0. This shows that the combined measurement is consistent with the other input measurements of NNPDF-3.0.

The uncertainties for the combination are summarized in the table below. In this table, 'Data' denotes the uncertainties from the Afb measurement, and 'Pred' denotes the prediction uncertainties.

Source sin2θefflept sin2θW
Data: Measurement±0.00043 (stat) ±0.00041 (stat)
Data: Energy scale±0.00002 (syst) ±0.00002 (syst)
Data: Backgrounds±0.00003 (syst) ±0.00003 (syst)
Pred: QCD scales±0.00006 (syst) ±0.00007 (syst)
Pred: QCD PDFs±0.00016 (syst) ±0.00016 (syst)
Pred: Form factor ±0.00008 (syst)

The energy scale, resolution and background systematic uncertainties from the muon and electron measurements are uncorrelated. As the electron and muon QCD systematic uncertainties are correlated, they are derived directly from the joint-comparison results.

The results of the combination are summarized below.

where the first uncertainty is the statistical uncertainty, and the second is the systematic uncertainty. All systematic uncertainties are included and combined in quadrature.

The corresponding sin2θefflept measurements from LEP-1/SLD [Phys. Rep. 427, 257 (2006)], and from the the Afb measurements of D0 [PRL 115, 041801 (2015)] and CDF [PRD 89,072005 (2014)] using their full Run II datasets are:

The LEP-1 and SLD values are standard model analysis of Z-pole results. The Al measurement corresponds to pure leptonic couplings. The Tevatron Drell-Yan results are produced mainly from light quarks and correspond to lepton-quark couplings. Graphical summaries of the result and comparison with other measurements are shown below.
Comparison of sin2θefflept that includes latest LHC results from CMS [ Phys. Rev. D84 112002, 2011 ], ATLAS [ J. High Energy Phys. 09 (2015) 049 ], and LHCb [ J. High Energy Phys. 11 (2015) 190 ]. The LEP-1+SLD Z-pole entry is the combination of their six Z-pole measurements.

The inferred value of sin2θW is usually expressed as an indirect W-boson mass value. There are other indirect W-boson mass results, including those from LEP-1 and SLD which are from standard model fits to Z-pole measurements with the top quark mass, and there are direct W-mass measurements from the Tevatron and LEP-2 [Phys. Rev. D86, 010001 (2012): PDG W mass review, 2015 update].
All measurements except for 'TeV and LEP-2' are indirect W-mass measurements that use the standard model (on-shell scheme). NuTeV is the neutrino neutral current measurement [ PRL 88, 091802 (2002); PRL 90, 239902(E) (2003) ] from the Tevatron.